WEBVTT

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Howdy Star Gazers and welcome to this episode

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of Star Trails. Drew here and I'll be your guide

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to the night sky for the week starting July the

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6th through the 12th. This week we answer some

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listener mail and explore the mystery of mass.

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A big full moon looms low on the horizon, and

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we take a detour into the icy reaches of our

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solar system, where relics of the early universe

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hide away in the darkness. Whether you're tuning

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in from the backyard, the balcony, or just your

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imagination, I'm glad you're here. So find a

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cozy spot, let your eyes adjust, and let's see

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what the sky holds for us this week. Before we

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get into the night sky this week, I'd like to

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kick off this episode with a listener question,

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and this one really hits the sweet spot. Simple

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on the surface, but it opens the door to something

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surprisingly deep. Last week, Dale from Omaha

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wrote, Can you explain mass? I don't understand

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how mass is calculated or what that means. I've

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heard astrophysicists say two planets are the

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same size but have different masses. A simple

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explanation would be greatly appreciated. Dale,

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first off, thanks for writing in with this question,

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and I know you asked for a simple explanation,

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and I intend to provide one, but mass, although

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a reasonably straightforward concept in and of

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itself, is connected to some of the real mysteries

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of astrophysics and the workings of the universe.

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I'll get into a few of those in a moment, but

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let's first figure out what's going on at the

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most basic level. Mass is essentially how much

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stuff is packed into something. It's not about

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how big something looks, it's about how much

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material is actually in there. Think about two

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identical suitcases. One is filled with clothes,

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The other is packed with bricks. They take up

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the same space, but the one with bricks is a

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lot heavier. That's because it has more mass.

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Astronomers talk about mass all the time. Just

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like your question, two planets can be the same

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size, but one can have more mass. That means

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one is denser. Maybe it has a larger metal core

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or more rock and less gas. Same outside dimensions,

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but more weight on the inside. Let's consider

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Earth's planetary sister, Venus. Both Earth and

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Venus are roughly the same size, but Earth has

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more mass thanks to its larger metallic core.

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Let's take another example. Because it's summer,

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let's consider a beach ball compared to a bowling

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ball, maybe a good 16 -pounder. The beach ball

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is very light, but much larger than the bowling

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ball. The beach ball contains mostly air, while

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the bowling ball is filled with, well, whatever

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bowling balls are made of, dense resin or plastics,

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I assume. It's that density that matters, rather

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than the size. And density is what determines

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mass. Now, here's where things start to become

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fascinating. Let's shrink ourselves down to the

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molecular level. If you were to stand next to

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a beach ball and a bowling ball at this tiny

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size, you'd feel a gravitational pull towards

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the bowling ball. Mass is directly tied to gravity.

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The more mass something has, the stronger its

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gravitational pull. Earth pulls harder than the

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moon because it has more mass. The Sun keeps

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the planets in orbit because it's massive, not

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just in size, as the term is often used, but

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in actual weight. In astronomy, we can't weigh

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things directly, so we figure out mass by watching

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how objects move. For example, how fast a moon

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orbits a planet. That motion tells us how much

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gravity there is, and gravity tells us the mass.

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Now let's get weird. Mass accounts for some of

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the most fascinating phenomena in the universe,

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including one of the most extreme, black holes.

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These are the ultimate examples of mass and gravity

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gone wild. A black hole forms when a giant star

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collapses and all that mass gets squeezed into

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an incredibly tiny space. Imagine taking something

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more massive than the sun and cramming it into

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something the size of a city or smaller. The

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result is unbelievably dense. Now remember, gravity

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depends on mass, and our distance to an object

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alters how much gravity we experience. Because

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black holes are so compact, you can get extremely

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close to them. But if you get too close, you

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get sucked in, and there's no turning back. The

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gravity near them is so strong that even light

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can't escape. That's why they're black. If, purely

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as a thought experiment, our sun turned into

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a black hole, Earth would keep orbiting just

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like it does now, same mass, same distance. But

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if you flew close to that black hole, you'd cross

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a point of no return, where gravity takes over

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and there's no way back. We've understood the

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relationship between mass and gravity for a while.

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This was Isaac Newton's great breakthrough, later

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expanded by Einstein and his theories of relativity

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and space -time. Einstein also taught us that

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energy and mass are basically interchangeable.

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That, of course, is his famous equation E equals

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mc squared. But interestingly, we don't really

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know why mass affects gravity. This is one of

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the real unsolved mysteries of the universe.

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We just know that it does and that we can directly

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observe its effect. There are some interesting

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theories, gravitons for instance, particles that

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somehow influence gravity. There are string theories

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and theories based on that energy to mass relationship,

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but so far we just don't really know. But we

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do know what mass is and we know it shapes gravity.

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motion, orbits, and the entire cosmic dance.

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I know we went down a bit of a rabbit hole there,

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but hopefully we answered the question. If anyone

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out there listening has a question or a topic

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they'd like for me to cover, just visit our website,

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StarTrails .Show, and hit the contact link. Dale,

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thanks so much for writing in. The night sky

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is fairly quiet this week, and it will be dominated

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by the upcoming full moon. On Thursday, we're

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treated to the full buck moon rising in the evening

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sky. The buck moon is the traditional name given

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to July's full moon. It comes from, you guessed

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it, Native American traditions, named after the

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time of year when male deer began to grow their

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new antlers. It's a moment that marks high summer,

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and this year's buck moon has a little extra

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drama. Because it's rising low on the horizon,

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we'll experience what's known as the moon illusion.

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That trick of the eye where the moon looks huge

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when it's near the horizon, especially just after

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it rises. Our brains compare it to nearby objects

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like trees or rooftops, and we perceive it as

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being much larger. It's a gorgeous effect, and

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one of the best full moons of the year to photograph

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if you have clear skies in your area. Now onto

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the planets. Mercury is hanging out low in the

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west -northwest just after sunset around magnitude

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.3. Best seen early this week if you have a clear

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view of the horizon. Mars is hanging out in the

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west, still reddish but fading into the twilight.

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Saturn and Neptune are up in Pisces, rising late

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and sticking around into the night. Over in the

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predawn sky, Venus is bright and unmistakable

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in the east. Later in the week, it's joined by

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a faint Uranus hiding in Taurus. As always, you'll

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need a scope or good binoculars to spot Uranus

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and Neptune. It's still early, but meteor season

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is just around the corner. The Alpha Capra cornids

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begin trickling in this week. Slow moving fireballs,

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best later in July. And if you're a Perseid fan,

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we're only about a week away from the start of

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that shower's long lead up. Have you ever considered

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how far our solar system extends from the sun?

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In this episode, we're taking a little detour

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beyond the outer planets into the frozen frontiers

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of our solar system. We'll explore two of the

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most mysterious regions we've never actually

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seen with our own eyes, the Kuiper Belt and the

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Oort Cloud. These are the deep freeze zones of

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the cosmos, full of ancient icy leftovers, silent

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travelers, and even the occasional supersized

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comet. Let's start with the one closer to us.

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The Kuiper Belt, named after the Dutch -American

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astronomer Gerard Kuiper, is a ring of icy bodies

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orbiting the sun beyond Neptune, starting around

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30 astronomical units out. At that distance,

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sunlight is a pale glow, and the temperature

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is hundreds of degrees below zero. The Kuiper

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Belt is the solar system's icy junkyard. It's

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full of leftover material from when the planets

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formed about 4 .6 billion years ago. We're talking

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rocks, frozen gases, chunks of water ice, and

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other elements that never made it into planets.

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It's also home to some famous objects. Pluto,

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of course, demoted from planet status in 2006,

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is proudly orbiting in the Kuiper Belt. Eris

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is slightly smaller than Pluto, but helped force

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that whole redefinition of what a planet is.

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Then there's Haumea, shaped like a football and

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spinning so fast it completes a rotation every

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four hours. And Machi Machi, another dwarf planet

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named after a Polynesian creator god. These icy

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worlds are known as Kuiper Belt Objects, or KBOs.

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Many of them have moons, some have strange orbits,

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and there are probably hundreds of thousands

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more we haven't seen yet. NASA's New Horizons

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mission flew past Pluto in 2015, revealing its

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icy mountains, nitrogen glaciers, and unexpected

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complexity. And then it kept going. sending back

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images of another KBO, Arakoth, a reddish snowman

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-shaped object about 21 miles long. That flyby

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in 2019 gave us our very first close -up of a

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true Kuiper Belt object. Now let's take a quick

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detour about comets, snowballs in space with

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glowing tails. Short period comets swing by the

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Sun every few decades and often come from the

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Kuiper Belt. Think of Comet Halley or Comet Temple

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Tuttle. These objects orbit in more or less the

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same plane as the planets, and their orbits are

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usually predictable. But then there are the weird

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ones, the comets with giant lopsided orbits that

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take millions of years to return. That brings

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us to our next destination. Far beyond the Kuiper

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belt, somewhere between 2 ,000 and 100 ,000 astronomical

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units from the Sun is a theoretical shell of

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icy bodies called the Oort cloud. Unlike the

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flat disc -shaped Kuiper belt, the Oort cloud

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is spherical. Imagine a vast snow globe surrounding

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our entire solar system, and inside that globe

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are potentially trillions of icy fragments. comets,

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planetesimals, ancient debris, left over from

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the very formation of the Sun. We've never directly

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seen the Oort cloud, it's just too far. But we

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know it's there because of those long period

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comets that suddenly appear from deep space on

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incredibly eccentric orbits. Comets like Hale

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-Bopp, which passed by in 1997 and won't return

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for another 2500 years. Another such visitor

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was comet C2012S1, which was hyped in 2013, but

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broke apart near the Sun. And more recently,

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there's a mega comet, and we mentioned this one

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last week. In 2021, astronomers Pedro Bernardinelli

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and Gary Bernstein spotted something strange

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in data from the Dark Energy Survey. A fuzzy,

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slow -moving object as wide as 85 miles across.

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That's bigger than some small moons. Named comet

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Bernardinelli -Bernstein, it's considered the

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largest comet nucleus ever discovered. It's not

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coming anywhere near Earth. At its closest approach

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in 2031, it'll still be out past Saturn. Even

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though we won't be able to see it with the naked

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eye, this comet is giving scientists a rare opportunity

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to study a pristine, early solar system object,

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probably untouched since the sun was born. That's

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like getting a piece of solar system history

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frozen in deep space for billions of years. These

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frozen regions are like the archives of the solar

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system. The Kuiper Belt and the Oort Cloud preserve

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the raw materials from the early days of planet

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building, before Earth had oceans or life or

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even before Jupiter finished forming. Some scientists

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believe that comets from these outer zones delivered

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water and organic molecules to the early Earth.

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Others are looking into whether Oort Cloud comets

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could help explain the odd tilt of Uranus or

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even the idea of a hypothetical Planet Nine lurking

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in the darkness. And that's our journey to the

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far edge of the Sun's influence. From Pluto's

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neighborhood to the Oort Cloud's distant reaches,

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the outer solar system is more than just empty

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space. It's a museum of frozen time. If the stars

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spoke to you this week or if a question's been

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on your mind, I'd love to hear it. Visit our

00:15:35.690 --> 00:15:39.350
website, StarTrails .Show, where you can contact

00:15:39.350 --> 00:15:43.129
me and explore past episodes. Be sure to follow

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us on Blue Sky and YouTube. Links are in the

00:15:46.509 --> 00:15:49.789
show notes. Until we meet again beneath the stars,

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clear skies, everyone.
